Several recent studies have reported differences invsini, abundance-condensation temperature trends and chromospheric activity between samples of stars with and without Doppler-detected planets. These findings have been disputed, and the status of these results remains uncertain. We evaluate these claims using additional published data and find support for all three. © 2011 The Author Monthly Notices of the Royal Astronomical Society © 2011 RAS.
CITATION STYLE
Gonzalez, G. (2011). Parent stars of extrasolar planets - XII. Additional evidence for trends withvsini, condensation temperature and chromospheric activity. Monthly Notices of the Royal Astronomical Society: Letters, 416(1). https://doi.org/10.1111/j.1745-3933.2011.01102.x
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